Search results for "parameter"

showing 10 items of 14056 documents

CCDC 817805: Experimental Crystal Structure Determination

2011

Related Article: M.Sarwar, A.M.Madalan, F.Lloret, M.Julve, M.Andruh|2011|Polyhedron|30|2414|doi:10.1016/j.poly.2011.06.011

Aqua-chloro-(22'-(propane-13-diylbis((nitrilo)methylylidene))-bis(6-methoxyphenolato))-iron(iii)Space GroupCrystallographyCrystal SystemCrystal StructureCell ParametersExperimental 3D Coordinates
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Interaction of methyltin(IV) compounds with carboxylate ligands. Part 2: Formation thermodynamic parameters, predictive relationships and sequesterin…

2008

Thermodynamic data of mono-, di- and tri-methyltin(IV)-carboxylate complexes (acetate, malonate, succinate, oxydiacetate, diethylenetrioxydiacetate, malate, citrate, 1,2,3-tricarballylate, 1,2,3,4-butanetetracarboxylate, 1,2,3,4,5,6-benzenehexacarboxylate) in aqueous solution are reported at t = 25 °C and I = 0 mol l−1. Thermodynamic parameters obtained were analysed to formulate empirical predictive relationships as a function of different parameters, such as the number of carboxylate groups of the ligand and the charge of the alkyltin(IV) cation. Sequestration diagrams of citrate and 1,2,3-tricarballylate towards alkyltin(IV) cations at different pH values are also reported and discussed.…

Aqueous solutionLigandempirical relationshipInorganic chemistrymethyltin(IV) complexeGeneral ChemistryCalorimetryMedicinal chemistryInorganic Chemistrychemistry.chemical_compoundspeciation in aqueous solutionMalonatechemistrythermodynamic parameterSettore CHIM/01 - Chimica AnaliticaCarboxylatethermodynamic parametersempirical relationshipsmethyltin(IV) complexes; thermodynamic parameters; calorimetry; empirical relationships; speciation in aqueous solutionmethyltin(IV) complexescalorimetry
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Conflicting needs of the thermal indoor environment of museums: In search of a practical compromise

2008

Thermal indoor microclimate conditions in museum buildings refer to two important requirements: the preservation of works of art and the comfort of visitors to these buildings and/or those working inside them. Unfortunately, different works of art have different internal parameters which render the management and control of the indoor thermal microclimate difficult. In this work the values proposed by various standards for the thermal environment of museum buildings have been revised. Moreover, the indoor microclimatic conditions relating to people's comfort have been described, with the aim of singling out possible common ranges for these parameters. With this aim, a useful simultaneousnes…

ArcheologyEngineeringArchitectural engineeringIndex (economics)Materials Science (miscellaneous)Compromisemedia_common.quotation_subjectControl (management)MicroclimateConservationindoor environmentSimultaneousness indexSpectroscopymedia_commonSettore ING-IND/11 - Fisica Tecnica AmbientaleMicroclimatic parameterbusiness.industryComfort indoorCultural heritageItalian standard ruleWork (electrical)Chemistry (miscellaneous)Cultural heritageWorks of art conservationbusinessGeneral Economics Econometrics and FinanceJournal of Cultural Heritage
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People comfort and artwork saving in museums: comparing indoor requisites

2009

In museums, environmental indoor conditions should, contemporaneously, preserve the exhibited works of art and ensure the comfort conditions for people. Unfortunately, human and artworks requirements are characterised by different values of the physical indoor parameters that, occasionally, could become conflicting. In the paper, these problems are addressed by means of a literature analysis, with a specific attention to thermal comfort conditions of people. The possibility of finding common ranges of values for both requisites is finally discussed. Some recent technical recommendations on the matter have also been considered for indicating some HVAC equipment and appliances to be adopted i…

Architectural engineeringEngineeringSettore ING-IND/11 - Fisica Tecnica Ambientalecomfort indoorbusiness.industrymuseum buildingThermal comfortworks of art conservationmicroclimatic parameterslaw.inventionConservationlawAir conditioningVentilation (architecture)HVACbusinessInternational Journal of Sustainable Design
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Diagnostics of Helium-Argon Arc Discharge Plasma Based on Spectral Line Shape Measurements

1999

Electron densities and ion (gas) temperatures on the axis of an arc discharge plasma, produced at atmospheric pressure in a gas mixture of 95% helium and 5% argon, are determined at two arc currents. The evaluation of both main plasma parameters is based on line shape measurements, the ion temperature on the Doppler broadening of selected ArII lines, while the electron density on the Stark broadening of the hydrogen Hp line which appear in the spectrum due to hydrogen traces in the applied gases. The significance of reliable plasma diagnostics for determination of atomic structure data is discussed.

ArgonMaterials sciencePlasma parametersGeneral Physics and Astronomychemistry.chemical_elementPlasmaSpectral line shapeElectric arcchemistryPhysics::Plasma PhysicsPlasma diagnosticsPhysics::Atomic PhysicsAtomic physicsHeliumDoppler broadeningActa Physica Polonica A
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Wronskian Addition Formula and Darboux-Pöschl-Teller Potentials

2013

For the famous Darboux-Pöschl-Teller equation, we present new wronskian representation both for the potential and the related eigenfunctions. The simplest application of this new formula is the explicit description of dynamics of the DPT potentials and the action of the KdV hierarchy. The key point of the proof is some evaluation formulas for special wronskian determinant.

Article SubjectWronskianlcsh:MathematicsGeneral MathematicsMathematics::Spectral TheoryEigenfunctionKdV hierarchylcsh:QA1-939Variation of parametersAction (physics)AlgebraKey pointNonlinear Sciences::Exactly Solvable and Integrable SystemsRepresentation (mathematics)MathematicsMathematical physicsJournal of Mathematics
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 9 Spectroscopic …

2012

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2012 RAS © 2012 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

AstrofísicaCosmology and GravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)Large-scale structure of Universe[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Cosmological parametersFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsEnergia fosca (Astronomia)Astrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Measurement of distancesObservacions astronòmiquesDark energy0103 physical sciencesobservations [Cosmology]Dark energy (Astronomy)010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics/dk/atira/pure/core/subjects/cosmologyDistance scaleCosmologia010308 nuclear & particles physicsCosmology: observationsFísicaAstronomy and AstrophysicsCosmology and Extragalactic AstrophysicsCosmologyMesurament de les distànciesSpace and Planetary Science[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsAstronomical observations
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy…

2014

We present a one per cent measurement of the cosmic distance scale from the detections of the baryon acoustic oscillations in the clustering of galaxies from the Baryon Oscillation Spectroscopic Survey (BOSS), which is part of the Sloan Digital Sky Survey III (SDSS-III). Our results come from the Data Release 11 (DR11) sample, containing nearly one million galaxies and covering approximately $8\,500$ square degrees and the redshift range $0.2<z<0.7$. We also compare these results with those from the publicly released DR9 and DR10 samples. Assuming a concordance $\Lambda$CDM cosmological model, the DR11 sample covers a volume of 13\,Gpc${}^3$ and is the largest region of the Universe ever su…

AstrofísicaCosmology and GravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Cosmic microwave backgroundDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsdistance scaleAstrophysics01 natural sciencesObservacions astronòmiques0103 physical sciencesQB Astronomycosmological parametersdark energy010303 astronomy & astrophysicsQCSTFCAstrophysics::Galaxy AstrophysicsQBPhysics/dk/atira/pure/core/subjects/cosmologyCosmologia010308 nuclear & particles physicsAngular diameter distanceAstrophysics::Instrumentation and Methods for AstrophysicsSpectral densityRCUKAstronomy and AstrophysicsEspectroscòpia de microonesGalaxyRedshiftobservations [cosmology]CosmologyBaryonQC Physics13. Climate actionSpace and Planetary ScienceMicrowave spectroscopyBaryon acoustic oscillationslarge-scale structure of UniverseAstrophysics - Cosmology and Nongalactic AstrophysicsAstronomical observations
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Cosmological bounds on neutrino statistics

2018

We consider the phenomenological implications of the violation of the Pauli exclusion principle for neutrinos, focusing on cosmological observables such as the spectrum of Cosmic Microwave Background anisotropies, Baryon Acoustic Oscillations and the primordial abundances of light elements. Neutrinos that behave (at least partly) as bosonic particles have a modified equilibrium distribution function that implies a different influence on the evolution of the Universe that, in the case of massive neutrinos, can not be simply parametrized by a change in the effective number of neutrinos. Our results show that, despite the precision of the available cosmological data, only very weak bounds can …

AstrofísicaCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaCosmic microwave backgroundFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsNeutrino properties01 natural sciencesPartícules (Física nuclear)symbols.namesakePauli exclusion principleHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesis0103 physical sciencesStatisticsAnisotropy010303 astronomy & astrophysicsPhysicsCosmologia010308 nuclear & particles physicsBig bang nucleosynthesisSpectrum (functional analysis)High Energy Physics::PhenomenologyObservableAstronomy and AstrophysicsCosmological neutrinos neutrino properties big bang nucleosynthesis cosmological parameters from CMBRCosmological parameters from CMBRHigh Energy Physics - Phenomenologysymbolsastro-ph.COBig bang nucleosynthesis; Cosmological neutrinos; Cosmological parameters from CMBR; Neutrino properties; astro-ph.CO; astro-ph.CO; High Energy Physics - Phenomenology; Astronomy and AstrophysicsCosmological neutrinosHigh Energy Physics::ExperimentBaryon acoustic oscillationsNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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Cosmological parameters degeneracies and non-Gaussian halo bias

2010

We study the impact of the cosmological parameters uncertainties on the measurements of primordial non-Gaussianity through the large-scale non-Gaussian halo bias effect. While this is not expected to be an issue for the standard Lambda CDM model, it may not be the case for more general models that modify the large-scale shape of the power spectrum. We consider the so-called local non-Gaussianity model, parametrized by the f(NL) non-Gaussianity parameter which is zero for a Gaussian case, and make forecasts on f(NL) from planned surveys, alone and combined with a Planck CMB prior. In particular, we consider EUCLID- and LSST-like surveys and forecast the correlations among f(NL) and the runni…

AstrofísicaCúmuls de galàxiesParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundFOS: Physical sciencesGalaxy clustersAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesPower spectrumsymbols.namesake0103 physical sciencesPlanck010303 astronomy & astrophysicsRedshift surveysPhysicsSpectral indexCosmological parameters from LSSCosmologiaClusters of galaxies010308 nuclear & particles physicsEquation of state (cosmology)Order (ring theory)Spectral densityAstronomy and AstrophysicsCosmologyHubble volumeDark energysymbolsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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